The theory of the hot electron microbolometer proposed by Nahum et al.
assumed that the photon energy is thermalized in the electrons in the
Cu absorber before relaxing to the lattice. Since the photons initial
ly excite individual electrons to HBAR omega much greater than k(B)T,
however, direct relaxation of these hot electrons to phonons must also
be considered, Theoretical estimates suggest that this extra relaxati
on channel increases the effective thermal conductance for HBAR omega
much greater than k(B)T and influences bolometer noise, Calculations o
f these effects are presented which predict very useful performance bo
th for ground-based and space-based astronomical photometry at millime
ter and submillimeter wavelengths.